English

SN2010U -- a Luminous Nova in NGC 4214

Solar and Stellar Astrophysics 2015-05-19 v1

Abstract

The luminosity, light curve, post--maximum spectrum, and lack of a progenitor on deep pre-outburst images suggest that SN 2010U was a luminous, fast nova. Its outburst magnitude is consistent with that for a fast nova using the Maximum Magnitude-Rate of Decline relationship for classical novae.

Keywords

Cite

@article{arxiv.1005.4356,
  title  = {SN2010U -- a Luminous Nova in NGC 4214},
  author = {Roberta M. Humphreys and Jose L. Prieto and Philip Rosenfield and L. Andrew Helton and Christopher S. Kochanek and K. Z. Stanek and Rubab Khan and Dorota Szczygiel and Karen Mogren and Robert A. Fesen and Dan Milisavljevic and Benjamin Williams and Jeremiah Murphy and Julianne Dalcanton and Karoline Gilbert},
  journal= {arXiv preprint arXiv:1005.4356},
  year   = {2015}
}

Comments

8 pages, 4 figures

R2 v1 2026-06-21T15:27:02.252Z